peer reviewedContext. Owing to its unusual location and its isolation, the nature of the high Galactic latitude O9.5 Vp object HD 93521 is still uncertain. Aims: We have collected X-ray and optical observations to characterize the star and its surroundings. Methods: X-ray images and spectra are analysed to search for traces of a recent star formation event around HD 93521 and to search for the signature of a possible compact companion. Optical echelle spectra are analysed with plane-parallel model atmosphere codes, assuming either a spherical star or a gravity darkened rotationally flattened star, to infer the effective temperature and surface gravity, and to derive the He, C, N and O abundances of HD 93521. Results: The X-ray images rev...
Context. The very young open cluster NGC 6383 centered on the O-star binary HD 159176 is an interest...
Three Galactic O-type stars belong to the rare class of Of? p objects: HD 108, HD 191612, and HD 148...
Context. Plaskett's star (HD 47 129) is a very massive O + O binary that belongs to the Mon OB2 asso...
Context. Owing to its unusual location and its isolation, the nature of the high Galactic latitude O...
The O9.5 Vp star HD 93521 is a well known non-radial pulsator located at a high Galactic latitude. T...
We present a new optical spectroscopic study of the O-type binary HD 165052 based on high-and interm...
peer reviewedContext. Oe stars possibly form an extension to higher temperatures of the Be phenomeno...
peer reviewedContext. A growing number of Be and Oe stars, named the γ Cas stars, are known for thei...
Context. Very young open clusters are ideal places to study the X-ray properties of a homogeneous po...
Aims. The line profile variability and photometric variability of the O9.5Vp star HD93521 are examin...
Aims: Following the advent of increasingly sensitive X-ray observatories, deep observations of early...
A new high-quality set of orbital parameters for the O-type spectroscopic binary HD 93205 has been o...
As the brightest O-type X-ray source in the Carina nebula, HD 93250 (O4 III(fc)) is X-ray overlumino...
peer reviewedWe present the analysis of an extensive set of high-resolution spectroscopic observatio...
Context. Very young open clusters are ideal places to study the X-ray properties of a homogeneous po...
Context. The very young open cluster NGC 6383 centered on the O-star binary HD 159176 is an interest...
Three Galactic O-type stars belong to the rare class of Of? p objects: HD 108, HD 191612, and HD 148...
Context. Plaskett's star (HD 47 129) is a very massive O + O binary that belongs to the Mon OB2 asso...
Context. Owing to its unusual location and its isolation, the nature of the high Galactic latitude O...
The O9.5 Vp star HD 93521 is a well known non-radial pulsator located at a high Galactic latitude. T...
We present a new optical spectroscopic study of the O-type binary HD 165052 based on high-and interm...
peer reviewedContext. Oe stars possibly form an extension to higher temperatures of the Be phenomeno...
peer reviewedContext. A growing number of Be and Oe stars, named the γ Cas stars, are known for thei...
Context. Very young open clusters are ideal places to study the X-ray properties of a homogeneous po...
Aims. The line profile variability and photometric variability of the O9.5Vp star HD93521 are examin...
Aims: Following the advent of increasingly sensitive X-ray observatories, deep observations of early...
A new high-quality set of orbital parameters for the O-type spectroscopic binary HD 93205 has been o...
As the brightest O-type X-ray source in the Carina nebula, HD 93250 (O4 III(fc)) is X-ray overlumino...
peer reviewedWe present the analysis of an extensive set of high-resolution spectroscopic observatio...
Context. Very young open clusters are ideal places to study the X-ray properties of a homogeneous po...
Context. The very young open cluster NGC 6383 centered on the O-star binary HD 159176 is an interest...
Three Galactic O-type stars belong to the rare class of Of? p objects: HD 108, HD 191612, and HD 148...
Context. Plaskett's star (HD 47 129) is a very massive O + O binary that belongs to the Mon OB2 asso...